As remarked earlier, several acc-SySt have been known for quite a
while. A few of them present emission lines bright enough to be
recognizable even on objective prism plates or low resolution optical
spectra. They are well epitomized by EG And, an M2III giant orbited every
481 days by a WD, whose accretion luminosity is a few 10\(^2\)  L\(_\odot \) 
[1]}.
